This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.72 12:00:25.01 +45:26:45.8
148.60941 69.05419 galactic UMa Second-epoch detections are separated by 1.3" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:00:25.01 +45:26:45.8 (user input) | T | P | (position from user input) J-Ks=0.548+/-0.026 (K)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 12:00:25.01 +45:26:45.8: 14.00 +/- 0.04 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 12:00:25.01 +45:26:45.8: 13.96 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 12 00 25.01 +45 26 45.8 12.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.03 11:56:58.11 +42:30:22.1
155.22431 71.04158 galactic UMa Second-epoch detections are separated by 1.2" and 6.1 pix
The object was found in VSX 1" Gaia DR3 768882541364754944
Type: ROT
# Max. Min./Amp. JD0 Period
12.590 G 12.600 G K
The object was not found in astcheck.
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:56:58.11 +42:30:22.1: 13.06 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:56:58.11 +42:30:22.1: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 56 58.11 +42 30 22.1 12.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 768882541364754944,2461324.9884,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 768882541364754944 20261011.4884 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.09 11:53:15.48 +42:01:27.4
157.78259 70.94489 galactic UMa Second-epoch detections are separated by 3.7" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:53:15.48 +42:01:27.4 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.540+/-0.028 (K)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:53:15.48 +42:01:27.4: 13.10 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:53:15.48 +42:01:27.4: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 53 15.48 +42 01 27.4 12.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.24 11:49:35.19 +41:06:53.4
161.25490 71.09944 galactic UMa Second-epoch detections are separated by 0.2" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:49:35.19 +41:06:53.4 (user input) | T | P | (position from user input) J-Ks=0.354+/-0.029 (G)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:49:35.19 +41:06:53.4: 13.19 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:49:35.19 +41:06:53.4: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 49 35.19 +41 06 53.4 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.23 11:15:12.01 +46:50:32.8
160.35521 62.68535 galactic UMa Second-epoch detections are separated by 1.9" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:15:12.01 +46:50:32.8 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.382+/-0.030 (G)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:15:12.01 +46:50:32.8: 13.23 +/- 0.03 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:15:12.01 +46:50:32.8: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 15 12.01 +46 50 32.8 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.26 12:02:31.28 +45:59:30.5
146.93419 68.78993 galactic UMa Second-epoch detections are separated by 1.3" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:02:31.28 +45:59:30.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 12:02:31.28 +45:59:30.5: 13.24 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 12:02:31.28 +45:59:30.5: 13.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 12 02 31.28 +45 59 30.5 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.29 11:58:15.36 +43:54:27.4
152.04722 70.09148 galactic UMa Second-epoch detections are separated by 2.3" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:58:15.36 +43:54:27.4 (user input) | T | P | (position from user input) J-Ks=0.277+/-0.032 (F)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:58:15.36 +43:54:27.4: 13.34 +/- 0.03 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:58:15.36 +43:54:27.4: 13.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 58 15.36 +43 54 27.4 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.43 11:57:33.55 +43:31:13.2
153.03814 70.32224 galactic UMa Second-epoch detections are separated by 1.0" and 5.8 pix
The object was found in VSX 1" Gaia DR3 769799808939981696
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.200 G 13.230 G F
The object was not found in astcheck.
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:57:33.55 +43:31:13.2: 13.40 +/- 0.03 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:57:33.55 +43:31:13.2: 13.30 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 57 33.55 +43 31 13.2 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 769799808939981696,2461324.9884,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 769799808939981696 20261011.4884 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.60 11:59:35.81 +45:17:19.5
149.18939 69.10520 galactic UMa Second-epoch detections are separated by 0.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:59:35.81 +45:17:19.5 (user input) | T | P | (position from user input) J-Ks=0.340+/-0.033 (G)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:59:35.81 +45:17:19.5: 13.70 +/- 0.03 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:59:35.81 +45:17:19.5: 13.62 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 59 35.81 +45 17 19.5 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.74 11:20:58.88 +49:13:48.9
155.10553 61.86410 galactic UMa Second-epoch detections are separated by 1.2" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:20:58.88 +49:13:48.9 (user input) | T | P | (position from user input) J-Ks=0.341+/-0.034 (G)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:20:58.88 +49:13:48.9: 13.78 +/- 0.04 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:20:58.88 +49:13:48.9: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 20 58.88 +49 13 48.9 12.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.43 11:51:11.96 +41:36:39.7
159.50862 70.97381 galactic UMa Second-epoch detections are separated by 0.0" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:51:11.96 +41:36:39.7 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.568+/-0.030 (K)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:51:11.96 +41:36:39.7: 13.74 +/- 0.04 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:51:11.96 +41:36:39.7: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 51 11.96 +41 36 39.7 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.78 11:18:42.19 +46:21:41.6
160.37220 63.45556 galactic UMa Second-epoch detections are separated by 1.0" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:18:42.19 +46:21:41.6 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.332+/-0.034 (G)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:18:42.19 +46:21:41.6: 13.76 +/- 0.05 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:18:42.19 +46:21:41.6: 14.16 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 18 42.19 +46 21 41.6 12.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.59 11:16:33.36 +46:52:00.2
160.00132 62.85298 galactic UMa Second-epoch detections are separated by 1.7" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:16:33.36 +46:52:00.2 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.425+/-0.028 (G)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:16:33.36 +46:52:00.2: 13.72 +/- 0.04 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:16:33.36 +46:52:00.2: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 16 33.36 +46 52 00.2 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.67 11:19:21.22 +46:08:41.8
160.59726 63.67811 galactic UMa Second-epoch detections are separated by 2.8" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J169.8386+46.1449 | 11:19:21.22 +46:08:41.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.286+/-0.031 (F)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:19:21.22 +46:08:41.8: 13.70 +/- 0.04 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:19:21.22 +46:08:41.8: 13.76 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 19 21.22 +46 08 41.8 12.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J169.8386+46.1449,2461324.9884,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J169.8386+46.1449 20261011.4884 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.72 11:18:51.39 +46:19:37.6
160.39588 63.49769 galactic UMa Second-epoch detections are separated by 1.5" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:18:51.39 +46:19:37.6 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.607+/-0.028 (K)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:18:51.39 +46:19:37.6: 13.68 +/- 0.04 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:18:51.39 +46:19:37.6: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 18 51.39 +46 19 37.6 12.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.62 11:56:08.43 +45:05:04.0
150.90828 68.92171 galactic UMa Second-epoch detections are separated by 1.0" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 773156755378989312 | 11:56:10.85 +45:04:26.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K0III 1962AJ.....67...37U NGP +45 45 J-Ks=0.373+/-0.033 (G)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:56:08.43 +45:05:04.0: 13.68 +/- 0.04 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:56:08.43 +45:05:04.0: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 56 08.43 +45 05 04.0 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 773156755378989312,2461324.9884,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 773156755378989312 20261011.4884 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.57 11:23:44.70 +48:36:34.1
155.39843 62.62099 galactic UMa Second-epoch detections are separated by 1.0" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:23:44.70 +48:36:34.1 (user input) | T | P | (position from user input) J-Ks=0.362+/-0.035 (G)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:23:44.70 +48:36:34.1: 13.67 +/- 0.04 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:23:44.70 +48:36:34.1: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 23 44.70 +48 36 34.1 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.56 12:01:58.76 +45:45:30.4
147.49699 68.93885 galactic UMa Second-epoch detections are separated by 2.5" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:01:58.76 +45:45:30.4 (user input) | T | P | (position from user input) J-Ks=0.364+/-0.029 (G)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 12:01:58.76 +45:45:30.4: 13.64 +/- 0.03 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 12:01:58.76 +45:45:30.4: 13.52 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 12 01 58.76 +45 45 30.4 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.63 11:23:50.64 +49:32:44.1
153.93499 61.97767 galactic UMa Second-epoch detections are separated by 2.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:23:50.64 +49:32:44.1 (user input) | T | P | (position from user input) J-Ks=0.402+/-0.038 (G)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:23:50.64 +49:32:44.1: 13.62 +/- 0.04 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:23:50.64 +49:32:44.1: 13.76 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 23 50.64 +49 32 44.1 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.62 11:18:41.90 +45:44:51.4
161.46490 63.83188 galactic UMa Second-epoch detections are separated by 2.1" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:18:41.90 +45:44:51.4 (user input) | T | P | (position from user input) J-Ks=0.334+/-0.031 (G)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:18:41.90 +45:44:51.4: 13.62 +/- 0.04 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:18:41.90 +45:44:51.4: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 18 41.90 +45 44 51.4 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.43 11:55:05.51 +43:02:46.9
154.96485 70.40668 galactic UMa Second-epoch detections are separated by 2.1" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:55:05.51 +43:02:46.9 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.546+/-0.030 (K)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:55:05.51 +43:02:46.9: 13.59 +/- 0.03 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:55:05.51 +43:02:46.9: 13.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 55 05.51 +43 02 46.9 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.66 11:21:55.73 +49:31:07.4
154.43877 61.77545 galactic UMa Second-epoch detections are separated by 1.0" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 790132493356782080 | 11:21:55.73 +49:31:07.4 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.371+/-0.037 (G)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:21:55.73 +49:31:07.4: 13.58 +/- 0.04 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:21:55.73 +49:31:07.4: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 21 55.73 +49 31 07.4 12.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 790132493356782080,2461324.9884,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 790132493356782080 20261011.4884 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.52 12:05:27.35 +47:47:09.7
143.39062 67.47446 galactic UMa Second-epoch detections are separated by 3.2" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:05:27.35 +47:47:09.7 (user input) | T | P | (position from user input) SpType: K0 (LAMOST DR5) J-Ks=0.614+/-0.028 (K)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 12:05:27.35 +47:47:09.7: 13.58 +/- 0.03 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 12:05:27.35 +47:47:09.7: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 12 05 27.35 +47 47 09.7 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.41 11:56:55.66 +43:03:11.3
154.17850 70.61574 galactic UMa Second-epoch detections are separated by 0.2" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:56:55.66 +43:03:11.3 (user input) | T | P | (position from user input) J-Ks=0.358+/-0.028 (G)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:56:55.66 +43:03:11.3: 13.54 +/- 0.03 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:56:55.66 +43:03:11.3: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 56 55.66 +43 03 11.3 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.59 11:18:27.35 +45:59:58.0
161.07176 63.64495 galactic UMa Second-epoch detections are separated by 2.4" and 5.7 pix
The object was found in VSX 2" Gaia DR3 788273906389961728
Type: ROT
# Max. Min./Amp. JD0 Period
13.870 G 13.900 G K
The object was not found in astcheck.
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:18:27.35 +45:59:58.0: 13.53 +/- 0.04 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:18:27.35 +45:59:58.0: 13.69 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 18 27.35 +45 59 58.0 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 788273906389961728,2461324.9884,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 788273906389961728 20261011.4884 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.60 11:25:00.02 +48:03:09.2
155.96773 63.15614 galactic UMa Second-epoch detections are separated by 2.4" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:25:00.02 +48:03:09.2 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.447+/-0.033 (G)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:25:00.02 +48:03:09.2: 13.52 +/- 0.03 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:25:00.02 +48:03:09.2: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 25 00.02 +48 03 09.2 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.31 11:56:50.88 +42:57:42.6
154.38697 70.67719 galactic UMa Second-epoch detections are separated by 0.6" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:56:50.88 +42:57:42.6 (user input) | T | P | (position from user input) J-Ks=0.452+/-0.026 (G)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:56:50.88 +42:57:42.6: 13.48 +/- 0.03 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:56:50.88 +42:57:42.6: 13.34 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 56 50.88 +42 57 42.6 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.58 11:15:33.82 +46:13:53.2
161.33812 63.10570 galactic UMa Second-epoch detections are separated by 0.7" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:15:33.82 +46:13:53.2 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.380+/-0.028 (G)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:15:33.82 +46:13:53.2: 13.46 +/- 0.03 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:15:33.82 +46:13:53.2: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 15 33.82 +46 13 53.2 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.44 11:55:00.82 +42:51:53.5
155.34950 70.53557 galactic UMa Second-epoch detections are separated by 2.9" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:55:00.82 +42:51:53.5 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.332+/-0.032 (G)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:55:00.82 +42:51:53.5: 13.47 +/- 0.03 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:55:00.82 +42:51:53.5: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 55 00.82 +42 51 53.5 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.32 11:55:07.18 +41:50:03.9
157.39723 71.31960 galactic UMa Second-epoch detections are separated by 1.3" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:55:07.18 +41:50:03.9 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.371+/-0.028 (G)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:55:07.18 +41:50:03.9: 13.44 +/- 0.03 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:55:07.18 +41:50:03.9: 13.32 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 55 07.18 +41 50 03.9 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.40 11:54:57.55 +43:09:17.1
154.81188 70.30824 galactic UMa Second-epoch detections are separated by 1.8" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:54:57.55 +43:09:17.1 (user input) | T | P | (position from user input) J-Ks=0.395+/-0.031 (G)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:54:57.55 +43:09:17.1: 13.43 +/- 0.03 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:54:57.55 +43:09:17.1: 13.32 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 54 57.55 +43 09 17.1 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.39 11:17:40.57 +46:30:21.7
160.36376 63.22715 galactic UMa Second-epoch detections are separated by 1.0" and 5.4 pix
The object was not found in VSX
The object was found in ASASSN-V 0" ASASSN-V J111740.58+463021.2
Type: EA
MeanMag 13.39 m Amp. 0.1 m Period 2.1379236 d
The object was not found in astcheck.
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:17:40.57 +46:30:21.7: 13.40 +/- 0.03 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:17:40.57 +46:30:21.7: 13.45 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 17 40.57 +46 30 21.7 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461324.9884,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261011.4884 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.32 12:06:48.45 +49:10:38.2
141.29770 66.32902 galactic UMa Second-epoch detections are separated by 4.5" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:06:48.45 +49:10:38.2 (user input) | T | P | (position from user input) J-Ks=0.348+/-0.031 (G)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 12:06:48.45 +49:10:38.2: 13.32 +/- 0.03 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 12:06:48.45 +49:10:38.2: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 12 06 48.45 +49 10 38.2 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.24 11:51:19.80 +41:47:10.4
159.07707 70.86709 galactic UMa Second-epoch detections are separated by 1.9" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:51:19.80 +41:47:10.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.359+/-0.033 (G)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:51:19.80 +41:47:10.4: 13.31 +/- 0.03 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:51:19.80 +41:47:10.4: 13.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 51 19.80 +41 47 10.4 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.39 11:57:26.96 +44:02:18.6
152.15513 69.89956 galactic UMa Second-epoch detections are separated by 1.8" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:57:26.96 +44:02:18.6 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.603+/-0.028 (K)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:57:26.96 +44:02:18.6: 13.30 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:57:26.96 +44:02:18.6: 13.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 57 26.96 +44 02 18.6 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.26 12:01:03.75 +45:17:06.1
148.59128 69.25104 galactic UMa Second-epoch detections are separated by 0.8" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:01:03.75 +45:17:06.1 (user input) | T | P | (position from user input) J-Ks=0.407+/-0.031 (G)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 12:01:03.75 +45:17:06.1: 13.25 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 12:01:03.75 +45:17:06.1: 13.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 12 01 03.75 +45 17 06.1 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.24 11:57:39.39 +43:13:20.1
153.54773 70.56734 galactic UMa Second-epoch detections are separated by 2.5" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J179.4107+43.2220 | 11:57:39.39 +43:13:20.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.440+/-0.028 (G)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:57:39.39 +43:13:20.1: 13.24 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:57:39.39 +43:13:20.1: 13.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 57 39.39 +43 13 20.1 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J179.4107+43.2220,2461324.9884,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J179.4107+43.2220 20261011.4884 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.18 11:59:35.15 +43:43:47.5
151.79277 70.37737 galactic UMa Second-epoch detections are separated by 1.7" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:59:35.15 +43:43:47.5 (user input) | T | P | (position from user input) J-Ks=0.783+/-0.028 (K)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:59:35.15 +43:43:47.5: 13.22 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:59:35.15 +43:43:47.5: 13.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 59 35.15 +43 43 47.5 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.12 11:54:50.02 +41:28:46.2
158.27970 71.54288 galactic UMa Second-epoch detections are separated by 0.6" and 6.1 pix
The object was found in VSX 7" Gaia DR3 768548805225691776
Type: ROT
# Max. Min./Amp. JD0 Period
12.460 G 12.500 G M
The object was not found in astcheck.
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:54:50.02 +41:28:46.2: 13.21 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:54:50.02 +41:28:46.2: 13.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 54 50.02 +41 28 46.2 12.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 768548805225691776,2461324.9884,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 768548805225691776 20261011.4884 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.19 11:59:38.16 +43:59:17.1
151.31875 70.17447 galactic UMa Second-epoch detections are separated by 0.3" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:59:38.16 +43:59:17.1 (user input) | T | P | (position from user input) J-Ks=0.302+/-0.034 (F)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:59:38.16 +43:59:17.1: 13.18 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:59:38.16 +43:59:17.1: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 59 38.16 +43 59 17.1 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 11.98 11:52:49.51 +41:04:59.8
160.00780 71.56197 galactic UMa Second-epoch detections are separated by 1.3" and 6.2 pix
The object was found in VSX 1" Gaia DR3 768524581610177024
Type: ROT
# Max. Min./Amp. JD0 Period
12.800 G 12.820 G K
The object was not found in astcheck.
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:52:49.51 +41:04:59.8: 13.14 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:52:49.51 +41:04:59.8: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 52 49.51 +41 04 59.8 12.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 768524581610177024,2461324.9884,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 768524581610177024 20261011.4884 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 11.97 11:58:41.30 +44:44:58.2
150.43009 69.45722 galactic UMa Second-epoch detections are separated by 0.5" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:58:41.30 +44:44:58.2 (user input) | T | P | (position from user input) J-Ks=0.358+/-0.028 (G)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:58:41.30 +44:44:58.2: 12.89 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:58:41.30 +44:44:58.2: 12.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 58 41.30 +44 44 58.2 12.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 11.88 11:55:08.97 +43:01:11.8
154.99178 70.43365 galactic UMa Second-epoch detections are separated by 0.7" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:55:08.97 +43:01:11.8 (user input) | T | P | (position from user input) J-Ks=0.313+/-0.028 (F)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:55:08.97 +43:01:11.8: 12.87 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:55:08.97 +43:01:11.8: 12.75 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 55 08.97 +43 01 11.8 11.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.88 11:18:47.75 +46:23:48.8
160.28804 63.44613 galactic UMa Second-epoch detections are separated by 0.9" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:18:47.75 +46:23:48.8 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.419+/-0.033 (G)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:18:47.75 +46:23:48.8: 14.08 +/- 0.06 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:18:47.75 +46:23:48.8: 14.18 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 18 47.75 +46 23 48.8 12.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4884 2461324.9884 12.54 11:50:49.56 +41:27:32.7
159.99178 71.03065 galactic UMa Second-epoch detections are separated by 0.6" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:50:49.56 +41:27:32.7 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.548+/-0.028 (K)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:50:49.56 +41:27:32.7: 13.86 +/- 0.04 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:50:49.56 +41:27:32.7: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 11.4884* 11 50 49.56 +41 27 32.7 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461324.9884,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.4884 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.79222760 22.02.2026 07:00:38.465 /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
First image: 2461093.79222760 22.02.2026 07:00:38.465 /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
Last image: 2461324.98863196 11.10.2026 11:43:27.801 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.24
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 2 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 5897
Objects passed selection criteria: 5892
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 3921.75
Average stars matched: 3703.25 (94.4285 %)
Memory usage VmPeak: 232648 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Oct 9 16:07:04 CDT 2026
VaST build number 1.0rc89-234-g1a8c12b2
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-09)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Oct 11 06:46:25 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.79222760 22.02.2026 07:00:38.465 /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
First image: 2461093.79222760 22.02.2026 07:00:38.465 /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
Last image: 2461324.98863196 11.10.2026 11:43:27.801 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 57
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -6.98
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 9 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 26975
Objects passed selection criteria: 26917
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 18781
Average stars matched: 17852.5 (95.0562 %)
Memory usage VmPeak: 252292 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Oct 9 16:07:04 CDT 2026
VaST build number 1.0rc89-234-g1a8c12b2
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-09)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Oct 11 06:47:13 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
SExtractor catalog cache: saved UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits.cat to cache
SExtractor catalog cache: saved UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461324.98807899
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits exists and is non-empty
wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits exists and is non-empty
wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits exists and is non-empty
wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits (1st reference image)
verification OK: wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
Image size: 941.8'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:59:59.840 +46:00:34.73 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits (1st new image)
verification OK: wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits
Image size: 942.1'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:59:38.903 +45:59:11.81 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:59:59.840 +46:00:34.73
Second-epoch image center 11:59:38.903 +45:59:11.81
Angular distance between the image centers 0.0648 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits (2nd new image)
verification OK: wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
Image size: 942.0'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:59:42.027 +45:59:23.49 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:59:59.840 +46:00:34.73
Second-epoch image center 11:59:42.027 +45:59:23.49
Angular distance between the image centers 0.0552 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 11:59:38.903 +45:59:11.81
Second-epoch second image center 11:59:42.027 +45:59:23.49
Angular distance between the image centers 0.00961 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits &> /tmp/tmp.AB58yx2saL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits &> /tmp/tmp.gmC3EPvEFA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits &> /tmp/tmp.8EJibx9mQu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits &> /tmp/tmp.ejBN7YnCkd
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
Calibrating the magnitude scale
Found non-empty wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits and wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits and wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits.wcscat
Found non-empty wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits and wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits.wcscat
The reference image (wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits) and catalog (wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits.wcscat) found
'wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits.wcscat' -> 'wcsmag.cat'
Read 6312 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 167.3583 to 191.9198 deg, Dec +39.8316 to +51.3978 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 167.3583 to 191.9198 deg, Dec 39.8316 to 51.3978 deg
Loaded 3936 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 2810 out of 2955 total matches.
Matched with Tycho-2 2955 out of 6312 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.929550
a=0.000000 b=1.000000 c=22.929550
From vast_summary.log: estimated ref. image limiting mag.: -7.24
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.69
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.69
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 6312 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 167.3583 to 191.9198 deg, Dec +39.8316 to +51.3978 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 167.3583 to 191.9198 deg, Dec 39.8316 to 51.3978 deg
Loaded 3936 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 2810 out of 2955 total matches.
Matched with Tycho-2 2955 out of 6312 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
Forced-photometry filter: calibrated wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits -> calib.txt_param_ref_wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits (aperture=6.5)
Read 6666 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 167.9142 to 192.3677 deg, Dec +40.1383 to +51.2474 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 167.9142 to 192.3677 deg, Dec 40.1383 to 51.2474 deg
Loaded 3769 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 2802 out of 2907 total matches.
Matched with Tycho-2 2907 out of 6666 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits
Forced-photometry filter: calibrated wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits -> calib.txt_param_ref_wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits (aperture=6.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
2.4 pix UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits
2.8 pix fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits
2.9 pix fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
Limiting magnitude estimates:
15.7 mag. UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
15.7 mag. UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits
12.3 mag. fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits
13.0 mag. fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
All-image limiting magnitude estimate: 12.3 (SNR ) 10.4 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.AB58yx2saL (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits' -> 'wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
WCS_IMAGE_NAME=wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
WCS-calibrated image found: wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
Checking if the catalog wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits.wcscat corresponding to the image wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits alredy exist and is non-empty...
Catalog wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits.wcscat corresponding to the image wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
WCS catalog name: wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=397, bad_region=0, passed=6312
Got 6312 stars (including 5911 good ones) from the SExtractor catalog wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits.wcscat
util/solve_plate_with_UCAC5 got 6312 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4846 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4837 matched stars entering correct_measured_positions(), 4837 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4837 matched stars entering correct_measured_positions(), 6312 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4846 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4837 matched stars entering correct_measured_positions(), 6312 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4837 matched stars entering correct_measured_positions(), 6312 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4837 stars left (next iteration limit 5320)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits N_match=4837 sigma_overall_arcsec=0.389 sigma_q1_arcsec=0.493 sigma_q2_arcsec=0.378 sigma_q3_arcsec=0.363 sigma_q4_arcsec=0.336 n_q1=1202 n_q2=1130 n_q3=1249 n_q4=1256 worst_quadrant_to_overall_ratio=1.268
The image catalog is written to wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits -region wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.gmC3EPvEFA (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits' -> 'wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits
WCS_IMAGE_NAME=wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits
WCS-calibrated image found: wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits
Checking if the catalog wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits.wcscat corresponding to the image wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits alredy exist and is non-empty...
Catalog wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits.wcscat corresponding to the image wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits
WCS catalog name: wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=353, bad_region=0, passed=6666
Got 6666 stars (including 6308 good ones) from the SExtractor catalog wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits.wcscat
util/solve_plate_with_UCAC5 got 6666 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.1 to 51.2)
Done reading UCAC5 zone files...
Matched 4840 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4832 matched stars entering correct_measured_positions(), 4832 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4832 matched stars entering correct_measured_positions(), 6666 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.1 to 51.2)
Done reading UCAC5 zone files...
Matched 4839 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4831 matched stars entering correct_measured_positions(), 6666 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4831 matched stars entering correct_measured_positions(), 6666 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4831 stars left (next iteration limit 5315)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits N_match=4831 sigma_overall_arcsec=0.321 sigma_q1_arcsec=0.277 sigma_q2_arcsec=0.362 sigma_q3_arcsec=0.335 sigma_q4_arcsec=0.313 n_q1=1233 n_q2=1155 n_q3=1237 n_q4=1206 worst_quadrant_to_overall_ratio=1.128
The image catalog is written to wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits -region wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.8EJibx9mQu (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits
WCS_IMAGE_NAME=wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits
WCS-calibrated image found: wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits
Checking if the catalog wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat corresponding to the image wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat corresponding to the image wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits
WCS catalog name: wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=53, bad_region=0, passed=1340
Got 1340 stars (including 1286 good ones) from the SExtractor catalog wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat
util/solve_plate_with_UCAC5 got 1340 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010468 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 1249 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1247 matched stars entering correct_measured_positions(), 1237 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1247 matched stars entering correct_measured_positions(), 1329 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 1249 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1247 matched stars entering correct_measured_positions(), 1330 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 1247 matched stars entering correct_measured_positions(), 1330 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 1247 stars left (next iteration limit 1371)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1247 robust_rms=10.834 arcsec worst_region_rms=26.700 arcsec outer_annulus_rms=26.700 arcsec
SIP_REFIT: SIP order 3 trial: matched=1247 robust_rms=0.504 arcsec worst_region_rms=0.583 arcsec outer_annulus_rms=0.570 arcsec
SIP_REFIT: SIP order 5 trial: matched=1247 robust_rms=0.308 arcsec worst_region_rms=0.425 arcsec outer_annulus_rms=0.379 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1247 robust_rms_before=1.149 arcsec robust_rms_before_corrected=0.300 arcsec robust_rms_after=0.308 arcsec worst_region_rms_before=0.402 worst_region_rms_after=0.425 outer_annulus_rms_before=1.232 outer_annulus_rms_after=0.379
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.402 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits worst_region_rms_kept=0.402 arcsec robust_rms_kept=0.300 arcsec matched=1247
WCS_QUALITY_DIAG: file=fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits N_match=1247 sigma_overall_arcsec=0.303 sigma_q1_arcsec=0.297 sigma_q2_arcsec=0.380 sigma_q3_arcsec=0.278 sigma_q4_arcsec=0.320 n_q1=371 n_q2=216 n_q3=427 n_q4=233 worst_quadrant_to_overall_ratio=1.252
The image catalog is written to wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits -region wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.ejBN7YnCkd (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
WCS_IMAGE_NAME=wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
WCS-calibrated image found: wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
Checking if the catalog wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits.wcscat corresponding to the image wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits.wcscat corresponding to the image wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
WCS catalog name: wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=65, bad_region=0, passed=1462
Got 1462 stars (including 1397 good ones) from the SExtractor catalog wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits.wcscat
util/solve_plate_with_UCAC5 got 1462 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010467 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 1357 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1355 matched stars entering correct_measured_positions(), 1341 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1355 matched stars entering correct_measured_positions(), 1444 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 1357 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1355 matched stars entering correct_measured_positions(), 1443 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 1355 matched stars entering correct_measured_positions(), 1443 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 1355 stars left (next iteration limit 1490)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1355 robust_rms=10.567 arcsec worst_region_rms=21.737 arcsec outer_annulus_rms=21.737 arcsec
SIP_REFIT: SIP order 3 trial: matched=1355 robust_rms=0.362 arcsec worst_region_rms=0.572 arcsec outer_annulus_rms=0.572 arcsec
SIP_REFIT: SIP order 5 trial: matched=1355 robust_rms=0.289 arcsec worst_region_rms=0.379 arcsec outer_annulus_rms=0.376 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1355 robust_rms_before=1.122 arcsec robust_rms_before_corrected=0.288 arcsec robust_rms_after=0.289 arcsec worst_region_rms_before=0.412 worst_region_rms_after=0.379 outer_annulus_rms_before=1.146 outer_annulus_rms_after=0.376
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.412 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits worst_region_rms_kept=0.412 arcsec robust_rms_kept=0.288 arcsec matched=1355
WCS_QUALITY_DIAG: file=fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits N_match=1355 sigma_overall_arcsec=0.287 sigma_q1_arcsec=0.279 sigma_q2_arcsec=0.374 sigma_q3_arcsec=0.254 sigma_q4_arcsec=0.298 n_q1=368 n_q2=240 n_q3=498 n_q4=249 worst_quadrant_to_overall_ratio=1.304
The image catalog is written to wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits -region wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits to local_wcs_cache/
'wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits' -> 'local_wcs_cache/wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits'
Saving the final (post-refit) wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits to local_wcs_cache/
'wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits' -> 'local_wcs_cache/wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits'
Saving the final (post-refit) wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits to local_wcs_cache/
'wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits' -> 'local_wcs_cache/wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits'
Saving the final (post-refit) wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits to local_wcs_cache/
'wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits' -> 'local_wcs_cache/wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits sigma_overall=0.389 worst_q_ratio=1.268
ref2=UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits sigma_overall=0.321 worst_q_ratio=1.128
new1=fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits sigma_overall=0.303 worst_q_ratio=1.252
new2=fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits sigma_overall=0.287 worst_q_ratio=1.304
reference average sigma_overall=0.355 worst_q_ratio=1.198
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308_astrometric_residuals.png (4837 matched stars from wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256_astrometric_residuals.png (4831 matched stars from wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409_astrometric_residuals.png (1247 matched stars from wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410_astrometric_residuals.png (1355 matched stars from wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.25 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits'
Saving fully-calibrated image wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits'
Preparing the HTML report for the field UMa-11-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field UMa-11-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
SExtractor catalog cache: saved UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits.cat to cache
SExtractor catalog cache: saved UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
Creating symlink local_wcs_cache/wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits
Creating symlink local_wcs_cache/wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits
Creating symlink local_wcs_cache/wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits exists and is non-empty
wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits exists and is non-empty
wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits exists and is non-empty
wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits (1st reference image)
verification OK: wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
Image size: 941.8'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:59:59.840 +46:00:34.73 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits (1st new image)
verification OK: wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits
Image size: 942.1'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:59:38.903 +45:59:11.81 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:59:59.840 +46:00:34.73
Second-epoch image center 11:59:38.903 +45:59:11.81
Angular distance between the image centers 0.0648 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits (2nd new image)
verification OK: wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
Image size: 942.0'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:59:42.027 +45:59:23.49 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:59:59.840 +46:00:34.73
Second-epoch image center 11:59:42.027 +45:59:23.49
Angular distance between the image centers 0.0552 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 11:59:38.903 +45:59:11.81
Second-epoch second image center 11:59:42.027 +45:59:23.49
Angular distance between the image centers 0.00961 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits &> /tmp/tmp.tB2ueCIp7x
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits &> /tmp/tmp.IXn4UfZcs4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits &> /tmp/tmp.ZZARO39ZeO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits &> /tmp/tmp.HbI4Yz7wAw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
Calibrating the magnitude scale
Found non-empty wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits and wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits and wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits.wcscat
Found non-empty wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits and wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits.wcscat
The reference image (wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits) and catalog (wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits.wcscat) found
'wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits.wcscat' -> 'wcsmag.cat'
Read 30576 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 167.2087 to 191.9198 deg, Dec +39.8316 to +51.4126 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 167.2087 to 191.9198 deg, Dec 39.8316 to 51.4126 deg
Loaded 3968 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 2678 out of 2956 total matches.
Matched with Tycho-2 2956 out of 30576 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.820300
a=0.000000 b=1.000000 c=22.820300
From vast_summary.log: estimated ref. image limiting mag.: -6.98
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.84
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.84
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 30576 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 167.2087 to 191.9198 deg, Dec +39.8316 to +51.4126 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 167.2087 to 191.9198 deg, Dec 39.8316 to 51.4126 deg
Loaded 3968 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 2678 out of 2956 total matches.
Matched with Tycho-2 2956 out of 30576 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
Forced-photometry filter: calibrated wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits -> calib.txt_param_ref_wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits (aperture=5.1)
Read 29946 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 167.8308 to 192.4263 deg, Dec +40.1383 to +51.2775 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 167.8308 to 192.4263 deg, Dec 40.1383 to 51.2775 deg
Loaded 3794 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 2685 out of 2906 total matches.
Matched with Tycho-2 2906 out of 29946 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits
Forced-photometry filter: calibrated wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits -> calib.txt_param_ref_wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits (aperture=5.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 52 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
2.3 pix UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits
2.8 pix fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits
2.8 pix fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
Limiting magnitude estimates:
15.8 mag. UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
15.9 mag. UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits
12.9 mag. fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits
13.4 mag. fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
All-image limiting magnitude estimate: 12.9 (SNR ) 12.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.tB2ueCIp7x (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits' -> 'wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
WCS_IMAGE_NAME=wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
WCS-calibrated image found: wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
Checking if the catalog wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits.wcscat corresponding to the image wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits alredy exist and is non-empty...
Catalog wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits.wcscat corresponding to the image wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits
WCS catalog name: wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=1202, bad_region=10, passed=30553
Got 30553 stars (including 29289 good ones) from the SExtractor catalog wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits.wcscat
util/solve_plate_with_UCAC5 got 30553 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4845 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4836 matched stars entering correct_measured_positions(), 4836 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4836 matched stars entering correct_measured_positions(), 30553 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4845 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4836 matched stars entering correct_measured_positions(), 30553 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4836 matched stars entering correct_measured_positions(), 30553 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4836 stars left (next iteration limit 5319)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits N_match=4836 sigma_overall_arcsec=0.369 sigma_q1_arcsec=0.472 sigma_q2_arcsec=0.368 sigma_q3_arcsec=0.345 sigma_q4_arcsec=0.328 n_q1=1198 n_q2=1128 n_q3=1256 n_q4=1254 worst_quadrant_to_overall_ratio=1.279
The image catalog is written to wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits -region wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.IXn4UfZcs4 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits' -> 'wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits
WCS_IMAGE_NAME=wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits
WCS-calibrated image found: wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits
Checking if the catalog wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits.wcscat corresponding to the image wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits alredy exist and is non-empty...
Catalog wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits.wcscat corresponding to the image wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits
WCS catalog name: wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=1201, bad_region=1, passed=29928
Got 29928 stars (including 28680 good ones) from the SExtractor catalog wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits.wcscat
util/solve_plate_with_UCAC5 got 29928 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.1 to 51.3)
Done reading UCAC5 zone files...
Matched 4844 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4837 matched stars entering correct_measured_positions(), 4837 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4837 matched stars entering correct_measured_positions(), 29928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.1 to 51.3)
Done reading UCAC5 zone files...
Matched 4844 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4836 matched stars entering correct_measured_positions(), 29928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4836 matched stars entering correct_measured_positions(), 29928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4836 stars left (next iteration limit 5320)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits N_match=4836 sigma_overall_arcsec=0.325 sigma_q1_arcsec=0.282 sigma_q2_arcsec=0.359 sigma_q3_arcsec=0.326 sigma_q4_arcsec=0.308 n_q1=1234 n_q2=1181 n_q3=1209 n_q4=1212 worst_quadrant_to_overall_ratio=1.106
The image catalog is written to wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits -region wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.ZZARO39ZeO (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits
WCS_IMAGE_NAME=wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits
WCS-calibrated image found: wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits
Checking if the catalog wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat corresponding to the image wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat corresponding to the image wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits
WCS catalog name: wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=120, bad_region=28, passed=7399
Got 7399 stars (including 7246 good ones) from the SExtractor catalog wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat
util/solve_plate_with_UCAC5 got 7399 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010468 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4742 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4728 matched stars entering correct_measured_positions(), 4728 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4728 matched stars entering correct_measured_positions(), 7399 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4742 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4728 matched stars entering correct_measured_positions(), 7399 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 4728 matched stars entering correct_measured_positions(), 7399 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 4728 stars left (next iteration limit 5200)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4728 robust_rms=11.988 arcsec worst_region_rms=28.117 arcsec outer_annulus_rms=28.117 arcsec
SIP_REFIT: SIP order 3 trial: matched=4728 robust_rms=0.762 arcsec worst_region_rms=0.924 arcsec outer_annulus_rms=0.921 arcsec
SIP_REFIT: SIP order 5 trial: matched=4728 robust_rms=0.625 arcsec worst_region_rms=0.819 arcsec outer_annulus_rms=0.737 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4728 robust_rms_before=1.298 arcsec robust_rms_before_corrected=0.631 arcsec robust_rms_after=0.625 arcsec worst_region_rms_before=0.844 worst_region_rms_after=0.819 outer_annulus_rms_before=1.395 outer_annulus_rms_after=0.737
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.844 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits worst_region_rms_kept=0.844 arcsec robust_rms_kept=0.631 arcsec matched=4728
WCS_QUALITY_DIAG: file=fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits N_match=4728 sigma_overall_arcsec=0.564 sigma_q1_arcsec=0.547 sigma_q2_arcsec=0.736 sigma_q3_arcsec=0.485 sigma_q4_arcsec=0.612 n_q1=1324 n_q2=824 n_q3=1605 n_q4=975 worst_quadrant_to_overall_ratio=1.306
The image catalog is written to wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits -region wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.HbI4Yz7wAw (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
WCS_IMAGE_NAME=wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
WCS-calibrated image found: wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
Checking if the catalog wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits.wcscat corresponding to the image wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits.wcscat corresponding to the image wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
WCS catalog name: wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=144, bad_region=32, passed=7889
Got 7889 stars (including 7700 good ones) from the SExtractor catalog wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits.wcscat
util/solve_plate_with_UCAC5 got 7889 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010467 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 4740 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4729 matched stars entering correct_measured_positions(), 4729 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4729 matched stars entering correct_measured_positions(), 7889 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 4740 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4728 matched stars entering correct_measured_positions(), 7889 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 4728 matched stars entering correct_measured_positions(), 7889 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 4728 stars left (next iteration limit 5201)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4728 robust_rms=11.206 arcsec worst_region_rms=25.526 arcsec outer_annulus_rms=25.526 arcsec
SIP_REFIT: SIP order 3 trial: matched=4728 robust_rms=0.693 arcsec worst_region_rms=0.865 arcsec outer_annulus_rms=0.865 arcsec
SIP_REFIT: SIP order 5 trial: matched=4728 robust_rms=0.597 arcsec worst_region_rms=0.766 arcsec outer_annulus_rms=0.707 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4728 robust_rms_before=1.238 arcsec robust_rms_before_corrected=0.606 arcsec robust_rms_after=0.597 arcsec worst_region_rms_before=0.797 worst_region_rms_after=0.766 outer_annulus_rms_before=1.301 outer_annulus_rms_after=0.707
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.797 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits worst_region_rms_kept=0.797 arcsec robust_rms_kept=0.606 arcsec matched=4728
WCS_QUALITY_DIAG: file=fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits N_match=4728 sigma_overall_arcsec=0.542 sigma_q1_arcsec=0.549 sigma_q2_arcsec=0.696 sigma_q3_arcsec=0.444 sigma_q4_arcsec=0.595 n_q1=1285 n_q2=835 n_q3=1654 n_q4=954 worst_quadrant_to_overall_ratio=1.286
The image catalog is written to wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits -region wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-42-40_20.00sec_-0.00C_LIGHTs_0409.fits
Saving fully-calibrated image wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_UMa-11-Q1b1x1_064407_TTUQ1b1x1_450117_yOgNfKWH/wcs_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410.fits
Preparing the HTML report for the field UMa-11-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:56:58.11 +42:30:22.1: 13.06 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:58:15.36 +43:54:27.4: 13.34 +/- 0.03 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:57:33.55 +43:31:13.2: 13.40 +/- 0.03 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:53:15.48 +42:01:27.4: 13.10 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:49:35.19 +41:06:53.4: 13.19 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 12:00:25.01 +45:26:45.8: 14.00 +/- 0.04 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:15:12.01 +46:50:32.8: 13.23 +/- 0.03 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 12:02:31.28 +45:59:30.5: 13.24 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:59:35.81 +45:17:19.5: 13.70 +/- 0.03 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:20:58.88 +49:13:48.9: 13.78 +/- 0.04 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:15:12.01 +46:50:32.8: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Forced photometry filter KEPT candidate at 11:15:12.01 +46:50:32.8: ref_mag=13.25 +/- 0.02 new_mean_mag=12.2382 delta=1.01 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:53:15.48 +42:01:27.4: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.01
Forced photometry filter KEPT candidate at 11:53:15.48 +42:01:27.4: ref_mag=13.00 +/- 0.01 new_mean_mag=12.0944 delta=0.91 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:58:15.36 +43:54:27.4: 13.24 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:56:58.11 +42:30:22.1: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry reference-image weighted average: 12.99 +/- 0.01
Forced photometry filter KEPT candidate at 11:58:15.36 +43:54:27.4: ref_mag=13.29 +/- 0.02 new_mean_mag=12.2642 delta=1.02 (need > 0.90)
Forced photometry filter KEPT candidate at 11:56:58.11 +42:30:22.1: ref_mag=12.99 +/- 0.01 new_mean_mag=11.9901 delta=1.00 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 12:00:25.01 +45:26:45.8: 13.96 +/- 0.04 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 12:02:31.28 +45:59:30.5: 13.14 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:49:35.19 +41:06:53.4: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.01
Forced photometry filter KEPT candidate at 12:02:31.28 +45:59:30.5: ref_mag=13.18 +/- 0.01 new_mean_mag=12.2685 delta=0.92 (need > 0.90)
Forced photometry reference-image weighted average: 13.98 +/- 0.03
Forced photometry filter KEPT candidate at 12:00:25.01 +45:26:45.8: ref_mag=13.98 +/- 0.03 new_mean_mag=12.7092 delta=1.27 (need > 0.90)
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:57:33.55 +43:31:13.2: 13.30 +/- 0.02 detection
Forced photometry filter KEPT candidate at 11:49:35.19 +41:06:53.4: ref_mag=13.15 +/- 0.02 new_mean_mag=12.2111 delta=0.94 (need > 0.90)
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Forced photometry filter KEPT candidate at 11:57:33.55 +43:31:13.2: ref_mag=13.35 +/- 0.02 new_mean_mag=12.4370 delta=0.91 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:59:35.81 +45:17:19.5: 13.62 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.02
Forced photometry filter KEPT candidate at 11:59:35.81 +45:17:19.5: ref_mag=13.66 +/- 0.02 new_mean_mag=12.6076 delta=1.05 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:20:58.88 +49:13:48.9: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.03
Forced photometry filter KEPT candidate at 11:20:58.88 +49:13:48.9: ref_mag=13.79 +/- 0.03 new_mean_mag=12.7852 delta=1.00 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:51:11.96 +41:36:39.7: 13.74 +/- 0.04 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:18:42.19 +46:21:41.6: 13.76 +/- 0.05 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:51:11.96 +41:36:39.7: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.03
Forced photometry filter KEPT candidate at 11:51:11.96 +41:36:39.7: ref_mag=13.72 +/- 0.03 new_mean_mag=12.4375 delta=1.28 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:18:42.19 +46:21:41.6: 14.16 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.04
Forced photometry filter KEPT candidate at 11:18:42.19 +46:21:41.6: ref_mag=13.88 +/- 0.04 new_mean_mag=12.8098 delta=1.07 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:16:33.36 +46:52:00.2: 13.72 +/- 0.04 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:19:21.22 +46:08:41.8: 13.70 +/- 0.04 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:18:51.39 +46:19:37.6: 13.68 +/- 0.04 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:16:33.36 +46:52:00.2: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Forced photometry filter KEPT candidate at 11:16:33.36 +46:52:00.2: ref_mag=13.67 +/- 0.03 new_mean_mag=12.5956 delta=1.08 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:19:21.22 +46:08:41.8: 13.76 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Forced photometry filter KEPT candidate at 11:19:21.22 +46:08:41.8: ref_mag=13.73 +/- 0.03 new_mean_mag=12.6950 delta=1.03 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:56:08.43 +45:05:04.0: 13.68 +/- 0.04 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:23:44.70 +48:36:34.1: 13.67 +/- 0.04 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:18:51.39 +46:19:37.6: 13.87 +/- 0.05 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 12:01:58.76 +45:45:30.4: 13.64 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.03
Forced photometry filter KEPT candidate at 11:18:51.39 +46:19:37.6: ref_mag=13.76 +/- 0.03 new_mean_mag=12.7178 delta=1.04 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:23:50.64 +49:32:44.1: 13.62 +/- 0.04 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:23:44.70 +48:36:34.1: 13.74 +/- 0.04 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:56:08.43 +45:05:04.0: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.03
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 12:01:58.76 +45:45:30.4: 13.52 +/- 0.03 detection
Forced photometry filter KEPT candidate at 11:23:44.70 +48:36:34.1: ref_mag=13.70 +/- 0.03 new_mean_mag=12.6411 delta=1.06 (need > 0.90)
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Forced photometry filter KEPT candidate at 11:56:08.43 +45:05:04.0: ref_mag=13.71 +/- 0.03 new_mean_mag=12.6049 delta=1.10 (need > 0.90)
Forced photometry reference-image weighted average: 13.57 +/- 0.02
Forced photometry filter KEPT candidate at 12:01:58.76 +45:45:30.4: ref_mag=13.57 +/- 0.02 new_mean_mag=12.5717 delta=1.00 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:23:50.64 +49:32:44.1: 13.76 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Forced photometry filter KEPT candidate at 11:23:50.64 +49:32:44.1: ref_mag=13.68 +/- 0.03 new_mean_mag=12.5858 delta=1.09 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:18:41.90 +45:44:51.4: 13.62 +/- 0.04 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:18:41.90 +45:44:51.4: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.03
Forced photometry filter KEPT candidate at 11:18:41.90 +45:44:51.4: ref_mag=13.58 +/- 0.03 new_mean_mag=12.6517 delta=0.93 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:55:05.51 +43:02:46.9: 13.59 +/- 0.03 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:21:55.73 +49:31:07.4: 13.58 +/- 0.04 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:55:05.51 +43:02:46.9: 13.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.02
Forced photometry filter KEPT candidate at 11:55:05.51 +43:02:46.9: ref_mag=13.52 +/- 0.02 new_mean_mag=12.4263 delta=1.09 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:21:55.73 +49:31:07.4: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Forced photometry filter KEPT candidate at 11:21:55.73 +49:31:07.4: ref_mag=13.60 +/- 0.03 new_mean_mag=12.6534 delta=0.94 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 12:05:27.35 +47:47:09.7: 13.58 +/- 0.03 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 12:05:27.35 +47:47:09.7: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.02
Forced photometry filter KEPT candidate at 12:05:27.35 +47:47:09.7: ref_mag=13.52 +/- 0.02 new_mean_mag=12.4922 delta=1.03 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:56:55.66 +43:03:11.3: 13.54 +/- 0.03 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:18:27.35 +45:59:58.0: 13.53 +/- 0.04 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:56:55.66 +43:03:11.3: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.02
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:25:00.02 +48:03:09.2: 13.52 +/- 0.03 detection
Forced photometry filter KEPT candidate at 11:56:55.66 +43:03:11.3: ref_mag=13.48 +/- 0.02 new_mean_mag=12.4259 delta=1.06 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:18:27.35 +45:59:58.0: 13.69 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Forced photometry filter KEPT candidate at 11:18:27.35 +45:59:58.0: ref_mag=13.60 +/- 0.03 new_mean_mag=12.5829 delta=1.01 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:25:00.02 +48:03:09.2: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.02
Forced photometry filter KEPT candidate at 11:25:00.02 +48:03:09.2: ref_mag=13.55 +/- 0.02 new_mean_mag=12.5975 delta=0.95 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:56:50.88 +42:57:42.6: 13.48 +/- 0.03 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:15:33.82 +46:13:53.2: 13.46 +/- 0.03 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:55:00.82 +42:51:53.5: 13.47 +/- 0.03 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:56:50.88 +42:57:42.6: 13.34 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Forced photometry filter KEPT candidate at 11:56:50.88 +42:57:42.6: ref_mag=13.40 +/- 0.02 new_mean_mag=12.3153 delta=1.09 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:15:33.82 +46:13:53.2: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.03
Forced photometry filter KEPT candidate at 11:15:33.82 +46:13:53.2: ref_mag=13.53 +/- 0.03 new_mean_mag=12.6039 delta=0.93 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:55:00.82 +42:51:53.5: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.02
Forced photometry filter KEPT candidate at 11:55:00.82 +42:51:53.5: ref_mag=13.44 +/- 0.02 new_mean_mag=12.4128 delta=1.03 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:55:07.18 +41:50:03.9: 13.44 +/- 0.03 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:55:07.18 +41:50:03.9: 13.32 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:54:57.55 +43:09:17.1: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Forced photometry filter KEPT candidate at 11:55:07.18 +41:50:03.9: ref_mag=13.37 +/- 0.02 new_mean_mag=12.3408 delta=1.03 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:17:40.57 +46:30:21.7: 13.40 +/- 0.03 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 12:06:48.45 +49:10:38.2: 13.32 +/- 0.03 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:54:57.55 +43:09:17.1: 13.32 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Forced photometry filter KEPT candidate at 11:54:57.55 +43:09:17.1: ref_mag=13.37 +/- 0.02 new_mean_mag=12.3781 delta=0.99 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:17:40.57 +46:30:21.7: 13.45 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Forced photometry filter KEPT candidate at 11:17:40.57 +46:30:21.7: ref_mag=13.42 +/- 0.02 new_mean_mag=12.4254 delta=1.00 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 12:06:48.45 +49:10:38.2: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Forced photometry filter KEPT candidate at 12:06:48.45 +49:10:38.2: ref_mag=13.34 +/- 0.02 new_mean_mag=12.3377 delta=1.00 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:51:19.80 +41:47:10.4: 13.31 +/- 0.03 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:51:19.80 +41:47:10.4: 13.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter KEPT candidate at 11:51:19.80 +41:47:10.4: ref_mag=13.22 +/- 0.02 new_mean_mag=12.1902 delta=1.03 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:57:26.96 +44:02:18.6: 13.30 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:57:26.96 +44:02:18.6: 13.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Forced photometry filter KEPT candidate at 11:57:26.96 +44:02:18.6: ref_mag=13.27 +/- 0.02 new_mean_mag=12.3717 delta=0.90 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 12:01:03.75 +45:17:06.1: 13.25 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 12:01:03.75 +45:17:06.1: 13.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.01
Forced photometry filter KEPT candidate at 12:01:03.75 +45:17:06.1: ref_mag=13.20 +/- 0.01 new_mean_mag=12.2498 delta=0.95 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:57:39.39 +43:13:20.1: 13.24 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:57:39.39 +43:13:20.1: 13.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.01
Forced photometry filter KEPT candidate at 11:57:39.39 +43:13:20.1: ref_mag=13.18 +/- 0.01 new_mean_mag=12.2226 delta=0.96 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:59:35.15 +43:43:47.5: 13.22 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:54:50.02 +41:28:46.2: 13.21 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:59:35.15 +43:43:47.5: 13.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.01
Forced photometry filter KEPT candidate at 11:59:35.15 +43:43:47.5: ref_mag=13.19 +/- 0.01 new_mean_mag=12.2010 delta=0.99 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:59:38.16 +43:59:17.1: 13.18 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:54:50.02 +41:28:46.2: 13.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.01
Forced photometry filter KEPT candidate at 11:54:50.02 +41:28:46.2: ref_mag=13.12 +/- 0.01 new_mean_mag=12.0907 delta=1.03 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:59:38.16 +43:59:17.1: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.01
Forced photometry filter KEPT candidate at 11:59:38.16 +43:59:17.1: ref_mag=13.15 +/- 0.01 new_mean_mag=12.1969 delta=0.95 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:52:49.51 +41:04:59.8: 13.14 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:54:52.56 +41:50:20.7: 12.91 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:58:41.30 +44:44:58.2: 12.89 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:52:49.51 +41:04:59.8: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.01
Forced photometry filter KEPT candidate at 11:52:49.51 +41:04:59.8: ref_mag=13.10 +/- 0.01 new_mean_mag=11.9864 delta=1.11 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:54:52.56 +41:50:20.7: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.01
Forced photometry filter REJECTED candidate at 11:54:52.56 +41:50:20.7: ref_mag=12.88 +/- 0.01 new_mean_mag=12.0155 delta=0.86 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:58:41.30 +44:44:58.2: 12.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Forced photometry filter KEPT candidate at 11:58:41.30 +44:44:58.2: ref_mag=12.84 +/- 0.01 new_mean_mag=11.9391 delta=0.90 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:55:08.97 +43:01:11.8: 12.87 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:58:14.13 +43:53:05.0: 12.86 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:55:08.97 +43:01:11.8: 12.75 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Forced photometry filter KEPT candidate at 11:55:08.97 +43:01:11.8: ref_mag=12.80 +/- 0.01 new_mean_mag=11.8693 delta=0.93 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:58:14.13 +43:53:05.0: 12.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Forced photometry filter REJECTED candidate at 11:58:14.13 +43:53:05.0: ref_mag=12.80 +/- 0.01 new_mean_mag=11.9078 delta=0.90 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:57:36.15 +42:14:37.0: 12.84 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:56:10.31 +41:08:36.7: 12.76 +/- 0.02 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:57:36.15 +42:14:37.0: 12.77 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Forced photometry filter REJECTED candidate at 11:57:36.15 +42:14:37.0: ref_mag=12.80 +/- 0.01 new_mean_mag=11.9187 delta=0.88 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:56:10.31 +41:08:36.7: 12.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Forced photometry filter REJECTED candidate at 11:56:10.31 +41:08:36.7: ref_mag=12.70 +/- 0.01 new_mean_mag=11.8126 delta=0.89 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:18:47.75 +46:23:48.8: 14.08 +/- 0.06 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:18:47.75 +46:23:48.8: 14.18 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.05
Forced photometry filter KEPT candidate at 11:18:47.75 +46:23:48.8: ref_mag=14.12 +/- 0.05 new_mean_mag=12.9000 delta=1.22 (need > 0.90)
Forced photometry on wcs_UMa-11-Q1b1x1_2026-02-22_01-00-38_20.00sec_-15.00C_LIGHT_0308.fits at 11:50:49.56 +41:27:32.7: 13.86 +/- 0.04 detection
Forced photometry on wcs_UMa-11-Q1b1x1_2026-03-20_01-06-07_20.00sec_-14.90C_LIGHT_0256.fits at 11:50:49.56 +41:27:32.7: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.03
Forced photometry filter KEPT candidate at 11:50:49.56 +41:27:32.7: ref_mag=13.77 +/- 0.03 new_mean_mag=12.5226 delta=1.25 (need > 0.90)
Adding exclusion_list_local.txt__out01261.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01455.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02180.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02288.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02666.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03080.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03119.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03664.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04747.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05835.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06009.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06222.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06257.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06328.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06712.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07601.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08102.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08663.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08808.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09053.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10999.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12096.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12521.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12611.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13044.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13894.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14589.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16847.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17616.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20585.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20588.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21797.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21969.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22012.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22569.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22920.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23653.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25699.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26288.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27157.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29381.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29396.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29859.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 62s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 26s
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Considering the candidate 53168_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
The candidate 53168_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410 did not pass the final checks
**** FOUND 11:56:56.01 +49:29:45.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53293_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
The candidate 53293_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410 did not pass the final checks
**** FOUND 11:20:39.50 +45:00:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13044_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 13044_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 04747_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 04747_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 03664_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 03664_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 01455_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 01455_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 29381_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 29381_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 14589_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 14589_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 08663_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 08663_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 07601_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 07601_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 12611_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 12611_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 23653_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 23653_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 02666_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 02666_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 20588_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 20588_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 29396_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 29396_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 22569_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 22569_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 22012_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 22012_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 12096_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 12096_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 25699_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 25699_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 13894_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 13894_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 22996_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 22996_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 16847_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 16847_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 06328_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 06328_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 22920_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 22920_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 29859_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 29859_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 06257_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 06257_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 17616_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 17616_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 27157_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 27157_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 06009_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 06009_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 21969_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 21969_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 05835_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 05835_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 03080_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 03080_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 06640_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 06640_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 20585_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 20585_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 26288_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 26288_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 03119_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 03119_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 09053_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 09053_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 12521_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 12521_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 06712_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 06712_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 08102_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 08102_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02180_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 02180_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08808_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 08808_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01261_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 01261_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03101_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
The candidate 03101_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10999_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 10999_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 06222_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 06222_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
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Considering the candidate 08581_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
The candidate 08581_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04052_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
The candidate 04052_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01276_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
The candidate 01276_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21797_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 21797_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25706_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
The candidate 25706_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410 did not pass the final checks
**** FOUND 11:49:02.06 +49:11:36.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02288_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
Preparing report for the candidate 02288_fd_UMa-11-Q1b1x1_2026-10-11_06-43-27_20.00sec_-0.00C_LIGHTs_0410
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 92s
Prepared the HTML report for the field UMa-11-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
11:52:49.51 +41:04:59.8
11:49:35.19 +41:06:53.4
11:54:50.02 +41:28:46.2
11:50:49.56 +41:27:32.7
11:51:11.96 +41:36:39.7
11:55:07.18 +41:50:03.9
11:51:19.80 +41:47:10.4
11:53:15.48 +42:01:27.4
11:56:58.11 +42:30:22.1
11:55:00.82 +42:51:53.5
11:56:50.88 +42:57:42.6
11:55:08.97 +43:01:11.8
11:56:55.66 +43:03:11.3
11:55:05.51 +43:02:46.9
11:54:57.55 +43:09:17.1
11:57:39.39 +43:13:20.1
11:57:33.55 +43:31:13.2
11:59:35.15 +43:43:47.5
11:58:15.36 +43:54:27.4
11:59:38.16 +43:59:17.1
11:57:26.96 +44:02:18.6
11:58:41.30 +44:44:58.2
11:56:08.43 +45:05:04.0
12:01:03.75 +45:17:06.1
11:59:35.81 +45:17:19.5
12:00:25.01 +45:26:45.8
12:01:58.76 +45:45:30.4
12:02:31.28 +45:59:30.5
11:18:41.90 +45:44:51.4
11:18:27.35 +45:59:58.0
11:17:40.57 +46:30:21.7
11:18:42.19 +46:21:41.6
11:18:47.75 +46:23:48.8
11:15:33.82 +46:13:53.2
11:18:51.39 +46:19:37.6
11:19:21.22 +46:08:41.8
11:21:55.73 +49:31:07.4
11:23:50.64 +49:32:44.1
11:20:58.88 +49:13:48.9
11:23:44.70 +48:36:34.1
12:06:48.45 +49:10:38.2
11:25:00.02 +48:03:09.2
11:15:12.01 +46:50:32.8
11:16:33.36 +46:52:00.2
12:05:27.35 +47:47:09.7
########### Completed UMa-11-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
12:00:25.01 +45:26:45.8
11:56:58.11 +42:30:22.1
11:53:15.48 +42:01:27.4
11:49:35.19 +41:06:53.4
11:15:12.01 +46:50:32.8
12:02:31.28 +45:59:30.5
11:58:15.36 +43:54:27.4
11:57:33.55 +43:31:13.2
11:59:35.81 +45:17:19.5
11:20:58.88 +49:13:48.9
11:51:11.96 +41:36:39.7
11:18:42.19 +46:21:41.6
11:16:33.36 +46:52:00.2
11:19:21.22 +46:08:41.8
11:18:51.39 +46:19:37.6
11:56:08.43 +45:05:04.0
11:23:44.70 +48:36:34.1
12:01:58.76 +45:45:30.4
11:23:50.64 +49:32:44.1
11:18:41.90 +45:44:51.4
11:55:05.51 +43:02:46.9
11:21:55.73 +49:31:07.4
12:05:27.35 +47:47:09.7
11:56:55.66 +43:03:11.3
11:18:27.35 +45:59:58.0
11:25:00.02 +48:03:09.2
11:56:50.88 +42:57:42.6
11:15:33.82 +46:13:53.2
11:55:00.82 +42:51:53.5
11:55:07.18 +41:50:03.9
11:54:57.55 +43:09:17.1
11:17:40.57 +46:30:21.7
12:06:48.45 +49:10:38.2
11:51:19.80 +41:47:10.4
11:57:26.96 +44:02:18.6
12:01:03.75 +45:17:06.1
11:57:39.39 +43:13:20.1
11:59:35.15 +43:43:47.5
11:54:50.02 +41:28:46.2
11:59:38.16 +43:59:17.1
11:52:49.51 +41:04:59.8
11:58:41.30 +44:44:58.2
11:55:08.97 +43:01:11.8
11:18:47.75 +46:23:48.8
11:50:49.56 +41:27:32.7
###################################################################################
12:00:25.01 +45:26:45.8 -- not an asteroid (will add it to exclusion list)
11:56:58.11 +42:30:22.1 -- not an asteroid (will add it to exclusion list)
11:53:15.48 +42:01:27.4 -- not an asteroid (will add it to exclusion list)
11:49:35.19 +41:06:53.4 -- not an asteroid (will add it to exclusion list)
11:15:12.01 +46:50:32.8 -- not an asteroid (will add it to exclusion list)
12:02:31.28 +45:59:30.5 -- not an asteroid (will add it to exclusion list)
11:58:15.36 +43:54:27.4 -- not an asteroid (will add it to exclusion list)
11:57:33.55 +43:31:13.2 -- not an asteroid (will add it to exclusion list)
11:59:35.81 +45:17:19.5 -- not an asteroid (will add it to exclusion list)
11:20:58.88 +49:13:48.9 -- not an asteroid (will add it to exclusion list)
11:51:11.96 +41:36:39.7 -- not an asteroid (will add it to exclusion list)
11:18:42.19 +46:21:41.6 -- not an asteroid (will add it to exclusion list)
11:16:33.36 +46:52:00.2 -- not an asteroid (will add it to exclusion list)
11:19:21.22 +46:08:41.8 -- not an asteroid (will add it to exclusion list)
11:18:51.39 +46:19:37.6 -- not an asteroid (will add it to exclusion list)
11:56:08.43 +45:05:04.0 -- not an asteroid (will add it to exclusion list)
11:23:44.70 +48:36:34.1 -- not an asteroid (will add it to exclusion list)
12:01:58.76 +45:45:30.4 -- not an asteroid (will add it to exclusion list)
11:23:50.64 +49:32:44.1 -- not an asteroid (will add it to exclusion list)
11:18:41.90 +45:44:51.4 -- not an asteroid (will add it to exclusion list)
11:55:05.51 +43:02:46.9 -- not an asteroid (will add it to exclusion list)
11:21:55.73 +49:31:07.4 -- not an asteroid (will add it to exclusion list)
12:05:27.35 +47:47:09.7 -- not an asteroid (will add it to exclusion list)
11:56:55.66 +43:03:11.3 -- not an asteroid (will add it to exclusion list)
11:18:27.35 +45:59:58.0 -- not an asteroid (will add it to exclusion list)
11:25:00.02 +48:03:09.2 -- not an asteroid (will add it to exclusion list)
11:56:50.88 +42:57:42.6 -- not an asteroid (will add it to exclusion list)
11:15:33.82 +46:13:53.2 -- not an asteroid (will add it to exclusion list)
11:55:00.82 +42:51:53.5 -- not an asteroid (will add it to exclusion list)
11:55:07.18 +41:50:03.9 -- not an asteroid (will add it to exclusion list)
11:54:57.55 +43:09:17.1 -- not an asteroid (will add it to exclusion list)
11:17:40.57 +46:30:21.7 -- not an asteroid (will add it to exclusion list)
12:06:48.45 +49:10:38.2 -- not an asteroid (will add it to exclusion list)
11:51:19.80 +41:47:10.4 -- not an asteroid (will add it to exclusion list)
11:57:26.96 +44:02:18.6 -- not an asteroid (will add it to exclusion list)
12:01:03.75 +45:17:06.1 -- not an asteroid (will add it to exclusion list)
11:57:39.39 +43:13:20.1 -- not an asteroid (will add it to exclusion list)
11:59:35.15 +43:43:47.5 -- not an asteroid (will add it to exclusion list)
11:54:50.02 +41:28:46.2 -- not an asteroid (will add it to exclusion list)
11:59:38.16 +43:59:17.1 -- not an asteroid (will add it to exclusion list)
11:52:49.51 +41:04:59.8 -- not an asteroid (will add it to exclusion list)
11:58:41.30 +44:44:58.2 -- not an asteroid (will add it to exclusion list)
11:55:08.97 +43:01:11.8 -- not an asteroid (will add it to exclusion list)
11:18:47.75 +46:23:48.8 -- not an asteroid (will add it to exclusion list)
11:50:49.56 +41:27:32.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
11:15:12.01 +46:50:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:15:33.82 +46:13:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:16:33.36 +46:52:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:17:40.57 +46:30:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:18:27.35 +45:59:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:18:41.90 +45:44:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:18:42.19 +46:21:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:18:47.75 +46:23:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:18:51.39 +46:19:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:19:21.22 +46:08:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:20:58.88 +49:13:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:21:55.73 +49:31:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:23:44.70 +48:36:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:23:50.64 +49:32:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:25:00.02 +48:03:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:49:35.19 +41:06:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:50:49.56 +41:27:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:51:11.96 +41:36:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:51:19.80 +41:47:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:52:49.51 +41:04:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:53:15.48 +42:01:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:54:50.02 +41:28:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:54:57.55 +43:09:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:55:00.82 +42:51:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
11:55:05.51 +43:02:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:55:07.18 +41:50:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:55:08.97 +43:01:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:56:08.43 +45:05:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:56:50.88 +42:57:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:56:55.66 +43:03:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:56:58.11 +42:30:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:57:26.96 +44:02:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:57:33.55 +43:31:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:57:39.39 +43:13:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:58:15.36 +43:54:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:58:41.30 +44:44:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:59:35.15 +43:43:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
11:59:35.81 +45:17:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
11:59:38.16 +43:59:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:00:25.01 +45:26:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:01:03.75 +45:17:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:01:58.76 +45:45:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:02:31.28 +45:59:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:05:27.35 +47:47:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:06:48.45 +49:10:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
11:15:12.01 +46:50:32.8 -- not a known variable star
11:15:33.82 +46:13:53.2 -- not a known variable star
11:16:33.36 +46:52:00.2 -- not a known variable star
11:17:40.57 +46:30:21.7 -- a known variable star
11:18:27.35 +45:59:58.0 -- a known variable star
11:18:41.90 +45:44:51.4 -- not a known variable star
11:18:42.19 +46:21:41.6 -- not a known variable star
11:18:47.75 +46:23:48.8 -- not a known variable star
11:18:51.39 +46:19:37.6 -- not a known variable star
11:19:21.22 +46:08:41.8 -- not a known variable star
11:20:58.88 +49:13:48.9 -- not a known variable star
11:21:55.73 +49:31:07.4 -- not a known variable star
11:23:44.70 +48:36:34.1 -- not a known variable star
11:23:50.64 +49:32:44.1 -- not a known variable star
11:25:00.02 +48:03:09.2 -- not a known variable star
11:49:35.19 +41:06:53.4 -- not a known variable star
11:50:49.56 +41:27:32.7 -- not a known variable star
11:51:11.96 +41:36:39.7 -- not a known variable star
11:51:19.80 +41:47:10.4 -- not a known variable star
11:52:49.51 +41:04:59.8 -- a known variable star
11:53:15.48 +42:01:27.4 -- not a known variable star
11:54:50.02 +41:28:46.2 -- a known variable star
11:54:57.55 +43:09:17.1 -- not a known variable star
11:55:00.82 +42:51:53.5 -- not a known variable star
11:55:05.51 +43:02:46.9 -- not a known variable star
11:55:07.18 +41:50:03.9 -- not a known variable star
11:55:08.97 +43:01:11.8 -- not a known variable star
11:56:08.43 +45:05:04.0 -- not a known variable star
11:56:50.88 +42:57:42.6 -- not a known variable star
11:56:55.66 +43:03:11.3 -- not a known variable star
11:56:58.11 +42:30:22.1 -- a known variable star
11:57:26.96 +44:02:18.6 -- not a known variable star
11:57:33.55 +43:31:13.2 -- a known variable star
11:57:39.39 +43:13:20.1 -- not a known variable star
11:58:15.36 +43:54:27.4 -- not a known variable star
11:58:41.30 +44:44:58.2 -- not a known variable star
11:59:35.15 +43:43:47.5 -- not a known variable star
11:59:35.81 +45:17:19.5 -- not a known variable star
11:59:38.16 +43:59:17.1 -- not a known variable star
12:00:25.01 +45:26:45.8 -- not a known variable star
12:01:03.75 +45:17:06.1 -- not a known variable star
12:01:58.76 +45:45:30.4 -- not a known variable star
12:02:31.28 +45:59:30.5 -- not a known variable star
12:05:27.35 +47:47:09.7 -- not a known variable star
12:06:48.45 +49:10:38.2 -- not a known variable star
Found 39 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
45 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
exclusion_list_gaiadr2.txt NOT FOUND
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
11:15:12.01 +46:50:32.8
11:15:33.82 +46:13:53.2
11:16:33.36 +46:52:00.2
11:17:40.57 +46:30:21.7
11:18:27.35 +45:59:58.0
11:18:41.90 +45:44:51.4
11:18:42.19 +46:21:41.6
11:18:47.75 +46:23:48.8
11:18:51.39 +46:19:37.6
11:19:21.22 +46:08:41.8
11:20:58.88 +49:13:48.9
11:21:55.73 +49:31:07.4
11:23:44.70 +48:36:34.1
11:23:50.64 +49:32:44.1
11:25:00.02 +48:03:09.2
11:49:35.19 +41:06:53.4
11:50:49.56 +41:27:32.7
11:51:11.96 +41:36:39.7
11:51:19.80 +41:47:10.4
11:52:49.51 +41:04:59.8
11:53:15.48 +42:01:27.4
11:54:50.02 +41:28:46.2
11:54:57.55 +43:09:17.1
11:55:00.82 +42:51:53.5
11:55:05.51 +43:02:46.9
11:55:07.18 +41:50:03.9
11:55:08.97 +43:01:11.8
11:56:08.43 +45:05:04.0
11:56:50.88 +42:57:42.6
11:56:55.66 +43:03:11.3
11:56:58.11 +42:30:22.1
11:57:26.96 +44:02:18.6
11:57:33.55 +43:31:13.2
11:57:39.39 +43:13:20.1
11:58:15.36 +43:54:27.4
11:58:41.30 +44:44:58.2
11:59:35.15 +43:43:47.5
11:59:35.81 +45:17:19.5
11:59:38.16 +43:59:17.1
12:00:25.01 +45:26:45.8
12:01:03.75 +45:17:06.1
12:01:58.76 +45:45:30.4
12:02:31.28 +45:59:30.5
12:05:27.35 +47:47:09.7
12:06:48.45 +49:10:38.2
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461324.98807899 -observatory V36
14:37:47.00 -18:22:15.8 Mercury (0.0mag)
14:07:14.79 -20:55:34.4 Venus (-4.5mag)
08:40:08.77 +19:36:08.4 Mars (1.0mag)
09:34:25.47 +15:05:04.3 Jupiter (-1.9mag)
00:42:24.97 +01:36:44.4 Saturn (0.4mag)
04:12:04.23 +20:57:56.4 Uranus (5.6mag)
00:10:20.13 -00:25:40.6 Neptune (7.7mag)
20:24:10.77 -23:43:30.2 Pluto (14.5mag)
13:39:17.43 -15:08:44.2 Moon (-8.4mag)
-rw-r--r-- 1 apache apache 361 Oct 11 06:46 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461324.98807899:
09:34:19.72 +15:05:36.5 Io (6.1mag)
09:34:35.91 +15:04:07.2 Europa (6.2mag)
09:34:40.82 +15:03:40.2 Ganymede (5.6mag)
09:34:01.96 +15:07:12.0 Callisto (6.9mag)
09:34:10.45 +15:25:33.0 Himalia (15.6mag)
09:34:24.43 +15:05:10.3 Thebe (16.4mag)
09:33:00.44 +15:26:44.9 Elara (17.5mag)
09:36:51.34 +14:27:54.5 Pasiphae (17.8mag)
09:33:01.24 +15:32:10.3 Carme (18.8mag)
00:42:11.61 +01:36:56.0 Titan (8.2mag)
00:42:27.71 +01:36:40.6 Rhea (9.6mag)
00:41:54.48 +01:33:57.5 Iapetus (11.0mag)
00:42:09.42 +01:36:34.9 Hyperion (14.1mag)
00:40:44.38 +01:24:25.1 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Oct 11 06:46 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461324.98807899:
02:48:48.28 +21:19:59.5 JWST
17:29:49.41 +37:04:15.4 Chandra
14:38:10.31 -61:04:01.4 XMM-Newton
-rw-r--r-- 1 apache apache 96 Oct 11 06:46 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461324.98807899 -observatory V36
03:46:06.50 +20:11:56.6 17.1mag P/1996 R2 (Lagerkvist)
18:24:48.37 -33:29:40.1 14.7mag P/2010 H2 (Vales)
07:39:51.26 -72:24:31.7 17.2mag C/2014 UN271 (Bernardinelli-Bernstein)
06:15:51.21 +34:39:12.7 17.7mag C/2017 K2 (PANSTARRS)
07:30:13.44 +25:27:26.5 16.9mag C/2022 N2 (PANSTARRS)
09:01:59.41 +35:40:43.6 16.2mag C/2024 E1 (Wierzchos)
18:26:47.18 +41:31:16.3 17.4mag C/2024 J3 (ATLAS)
05:46:12.17 -13:35:28.5 16.6mag C/2024 T5 (ATLAS)
12:17:16.83 +15:59:11.2 16.2mag C/2025 V2 (Rankin)
13:51:05.12 -02:43:43.6 16.5mag C/2025 Y1 (ATLAS)
18:43:01.80 +65:10:45.2 15.8mag C/2026 A2 (Bok)
02:36:00.77 +43:16:27.9 17.8mag C/2026 B2 (Sun-Gao)
12:45:45.34 +14:16:15.6 17.7mag A/2026 E1
16:29:20.95 -21:13:18.2 12.9mag P/2026 R2 (Leonard)
00:26:46.37 +18:58:58.6 17.6mag 2P/Encke
22:58:23.01 -31:40:27.9 14.5mag 10P/Tempel
02:10:54.87 +38:43:16.9 16.8mag 11P/Tempel-Swift-LINEAR
12:11:18.08 -08:10:15.6 16.3mag 29P/Schwassmann-Wachmann
00:22:21.50 -08:52:26.5 15.6mag 65P/Gunn
07:35:55.10 +16:00:02.9 13.9mag 78P/Gehrels
02:59:57.75 +14:20:11.2 17.6mag 88P/Howell
07:39:18.78 +40:16:39.9 17.1mag 112P/Urata-Niijima
09:02:52.89 +14:06:42.8 17.8mag 114P/Wiseman-Skiff
11:41:13.51 +13:14:18.1 14.8mag 123P/West-Hartley
14:06:57.70 -32:14:39.3 17.8mag 124P/Mrkos
06:50:54.33 +19:18:16.2 15.6mag 128P/Shoemaker-Holt
21:38:39.69 +03:31:09.2 9.5mag 161P/Hartley-IRAS
10:18:44.30 +01:37:42.8 14.3mag 169P/NEAT
03:29:16.49 +04:35:10.0 14.8mag 220P/McNaught
06:03:37.55 +45:14:29.9 15.4mag 260P/McNaught
07:27:46.16 +25:36:56.2 17.9mag 266P/Christensen
09:56:20.43 +31:37:15.5 18.0mag 493P/LONEOS
-rw-r--r-- 1 apache apache 1.6K Oct 11 06:46 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
05:39:14.97 +51:06:11.70 ASASSN-26fk 2026-10-5.53 -3.9
02:49:03.98 -49:55:57.00 SN 2026adfy 2026-10-4.88 16.61
22:03:46.31 -11:07:57.70 AT2026adgn 2026-10-4.28 -2.56
15:03:12.98 +49:51:05.40 ASASSN-26fj 2026-10-2.06 15.91
08:07:27.96 -65:51:03.90 ASASSN-26fi 2026-10-1.36 15.82
21:02:34.66 +23:57:26.20 ASASSN-26fh 2026-10-1.27 15.94
20:00:16.62 +03:26:29.90 AT2026adfv 2026-10-1.3 16.42
00:08:42.74 -32:33:16.50 SN2026abhc 2026-09-29.15 15.57
21:02:30.26 -19:27:41.80 SN2026acxa 2026-09-29.13 14.65
04:39:17.45 -28:06:12.40 ASASSN-26fg 2026-09-23.25 15.73
05:25:07.80 +04:38:32.40 SN2026aajs 2026-09-21.32 17.04
19:56:12.67 +08:25:27.70 AT2026acgs 2026-09-18.14 15.84
00:02:34.07 +52:55:19.10 ASASSN-26ff 2026-09-16.43 15.37
23:44:33.18 +17:46:12.20 SN2026yjv 2026-09-15.38 18.32
16:21:12.24 +57:37:51.30 SN 2026aafh 2026-09-14.11 15.02
23:36:00.27 -19:28:18.00 SN 2026aaks 2026-09-14.44 16.89
16:35:24.86 -05:32:38.20 SN2026aasi 2026-09-12.99 16.58
16:46:08.71 +37:25:21.80 SN2026aafk 2026-09-13.25 17.4
23:48:37.86 +50:25:24.60 SN2026aafs 2026-09-13.47 17
21:20:27.02 +02:10:42.50 SN2026aagh -------
08:02:26.85 -24:37:44.10 ASASSN-26fe 2026-09-13.34 13.67
02:29:34.91 +23:06:56.30 SN2026aars 2026-09-12.27 16.93
02:47:25.52 -32:58:34.50 SN 2026znh 2026-09-9.92 16.26
04:59:14.53 -83:27:58.80 ASASSN-26fd 2026-09-9.11 17.27
17:52:06.79 -23:43:20.70 ASASSN-26fc 2026-09-8.79 12.14
03:52:53.26 -14:19:28.70 SN 2026zfw 2026-09-8 17.78
01:53:26.46 +10:07:25.10 SN2026aacj 2026-09-7.17 16.27
20:04:34.47 +62:38:38.10 SN2026zji 2026-09-7.14 15.87
22:37:05.59 +34:24:35.70 SN2026aaiv 2026-09-7.22 13.48
22:24:21.29 -10:25:31.60 ASASSN-26fb 2026-09-5.3 13.93
00:44:54.28 +41:33:10.50 AT2026aabo 2026-09-3.29 15.02
00:52:12.40 -58:22:08.60 SN 2026zhl 2026-08-31.92 16.51
19:53:57.87 +61:00:19.70 ASASSN-26fa 2026-08-31.18 14.63
00:21:50.96 -09:29:16.30 AT2026zwp 2026-08-31.41 15.59
19:45:06.20 +18:22:48.80 V488 2026-08-30.13 9.37
18:25:12.79 -22:25:29.10 V8055 2026-08-30 10.76
17:17:45.96 +64:31:40.10 ASASSN-26ez 2026-08-25.13 10.87
19:02:47.09 +58:08:21.00 AT2026zwo 2026-08-24.16 15.78
04:20:07.58 -42:26:59.90 AT2026zjy 2026-08-23.03 15.91
03:08:18.02 +11:54:46.50 SN2026ymb 2026-08-23.4 16.44
20:22:32.48 -50:45:14.30 SN2026yid 2026-08-22.82 15.13
04:24:28.39 -56:20:21.60 ASASSN-26ey 2026-08-20.02 15.55
16:46:37.81 -63:14:59.80 ASASSN-26ex 2026-08-18.78 3.63
21:28:47.85 +20:31:03.60 SN 2026sfn 2026-08-16.3 17.09
23:01:28.67 -61:00:39.00 SN 2026yib 2026-08-14.85 17.36
00:22:23.20 -32:16:02.70 SN 2026whu 2026-08-14.96 16.5
19:56:21.71 -37:24:19.90 ASASSN-26ew 2026-08-13.82 14.73
13:53:14.21 +00:26:52.00 SN 2026wkv 2026-08-10.12 15.83
05:21:07.61 +23:38:20.10 TCP J05210763+2338194 2026-08-10.59 9.34
01:28:20.49 +40:13:27.10 SN2026wpd 2026-08-9.34 16.37
23:47:50.87 +49:28:49.80 SN2026wjs 2026-08-9.35 17.12
16:03:20.92 +17:43:23.70 AT2026xau 2026-08-9.3 17.71
01:10:22.05 -09:34:08.50 SN2026weo 2026-08-7.46 15.76
00:56:54.35 -35:55:29.40 AT2026wdy 2026-08-5.05 16.08
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
-rw-r--r-- 1 apache apache 5.7K Oct 11 06:46 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
22:57:17.96 +47:07:41.8 TCP J22571796+4707418 2026-08-09.3289 14.3mag
09:13:38.17 +76:28:18.1 PSN J09133817+7628181 2026-08-09.8037 15.4mag
00:43:17.29 +41:26:48.6 PNV J00431729+4126486 2026-08-14.0920 16.8mag
00:42:52.82 +41:10:58.6 PNV J00425282+4110586 2026-08-17.7723 19.9mag
00:42:52.83 +41:10:59.6 PNV J00425283+4110596 2026-08-18.6119 19.3mag
18:25:12.76 -22:25:29.3 TCP J18251276-2225293 2026-08-19.1062 9.4mag
18:03:09.04 +12:18:14.0 TCP J18030904+1218140 2026-08-19.5199 14.9mag
19:45:06.48 +18:22:42.2 PNV J19450648+1822422 2026-08-25.1278 9.0mag
00:42:54.65 +41:22:59.3 PNV J00425465+4122593 2026-08-25.4712 18.9mag
00:42:50.38 +41:18:58.76 PNV J00425038+4118587 2026-09-04.1512 18.2mag
00:42:12.76 +41:16:28.4 PNV J00421276+4116284 2026-09-10.9176 18.67Cmag
17:52:06.80 -23:43:20.7 TCP J17520680-2343207 2026-09-08.7896 12.6mag
00:42:40.94 +41:15:37.1 PNV J00424094+4115371 2026-09-17.8925 18.3mag
08:49:20.13 -09:19:15.8 TCP J08492013-0919158 2026-09-18.4698 13.3mag
00:42:13.93 +41:16:35.6 PNV J00421393+4116356 2026-09-22.6597 19.66Cmag
18:14:01.58 +15:13:55.5 TCP J18140158+1513555 2026-09-24.4645 14.1mag
00:42:36.61 +41:13:50.5 TCP J00423661+4113505 2026-09-29.7462 17.4mag
22:03:46.29 -11:07:57.8 TCP J22034629-1107578 2026-09-29.7438 14.51Cmag
22:05:02.06 +20:49:01.2 TCP J22050206+2049012 2026-10-03.5715 17.13Cmag
00:38:15.01 +41:14:47.2 TCP J00381501+4114472 2026-10-08.5978 17.72Cmag
-rw-r--r-- 1 apache apache 191K Oct 11 06:46 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
22:00:29.980 +18:33:24.69 AT 2026acyi 2026-08-31.60 21.38
01:44:56.733 +00:38:32.49 AT 2026acyh 2026-09-21.88 22.21
01:45:25.068 +03:43:05.31 AT 2026acyg 2026-09-12.91 22.32
23:02:48.800 +03:40:01.33 AT 2026acyf 2026-08-31.80 21.75
05:44:27.090 +33:39:00.48 AT 2026acye 2026-09-25.43 18.62
06:12:59.365 -58:12:49.41 AT 2026acyd 2026-09-25.74 18.37
06:44:13.801 +10:23:30.61 AT 2026acyc 2026-09-24.45 17.58
21:50:55.698 -02:51:50.17 SN 2026acyb 2026-09-20.25 19.4497
17:12:55.487 +34:28:22.84 SN 2026acya 2026-09-22.17 19.6988
18:28:46.287 +43:53:39.30 AT 2026acxz 2026-09-22.18 19.7418
18:50:25.837 +51:48:48.31 AT 2026acxy 2026-09-26.14 19.507
17:29:04.550 +70:58:39.69 AT 2026acxx 2026-09-18.17 19.9857
18:36:38.362 +53:14:52.16 AT 2026acxw 2026-09-22.17 19.6863
03:16:13.837 +33:07:04.16 AT 2026acxv 2026-09-24.50 20.55
05:52:14.054 +15:53:08.19 AT 2026acxu 2026-09-22.43 20.8781
08:02:21.458 +24:05:52.06 AT 2026acxt 2026-09-24.51 19.9945
08:26:53.421 +00:01:31.92 AT 2026acxs 2026-09-24.52 18.9046
08:04:09.422 +26:03:07.21 AT 2026acxr 2026-09-16.52 20.3455
09:49:29.452 +22:28:47.85 AT 2026acxq 2026-09-24.52 18.9887
10:39:38.343 +25:39:08.54 AT 2026acxp 2026-09-24.53 18.7327
-rw-r--r-- 1 apache apache 89K Oct 11 06:46 tns_transients_list.txt
